Three Dimensional de Sitter Gravity and the Correspondence
Bruno Carneiro da Cunha

TL;DR
This paper explores three-dimensional de Sitter gravity, focusing on the boundary conformal symmetry and how boundary observables relate to spacetime properties like angular momentum, with insights into holonomies and isometry groups.
Contribution
It establishes a correspondence between gravity observables and boundary conformal weights, revealing that non-real weights indicate non-zero angular momentum in the spacetime.
Findings
Non-real conformal weights correspond to angular momentum
Holonomies and isometry groups play a role in the boundary correspondence
Insights into the structure of de Sitter space in three dimensions
Abstract
Certain aspects of three dimensional asymptotically de Sitter spaces are studied, with emphasis on the mapping between gravity observables and the representation of the conformal symmetry of the boundary. In particular, we show that non-real conformal weights for the boundary theory correspond to space-times that have non-zero angular momentum. Some miscellaneous results on the role of the holonomies and isometry groups are also presented.
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